Asymptotically flat, stable black hole solutions in Einstein--Yang-Mills--Chern-Simons theory

Details Asymptotically flat, stable black hole solutions in Einstein--Yang-Mills--Chern-Simons theory Asymptotically flat, stable black hole solutions in Einstein--Yang-Mills--Chern-Simons theory

2010-11-07

arxiv.org/abs/1011.1624v1

Phys.Rev.Lett.106:071101,2011

Physics

High Energy Physics

High Energy Physics - Theory

9 pages, 3 figures

Scientific paper

10.1103/PhysRevLett.106.071101

We construct finite mass, asymptotically flat black hole solutions in d=5 Einstein--Yang-Mills--Chern-Simons theory. Our results indicate the existence of a second order phase transition between Reissner-Nordstrom solutions and the non-Abelian black holes which generically are thermodynamically preferred. Some of the non-Abelian configurations are also stable under linear, spherically symmetric perturbations. In addition a solution in closed form describing an extremal black hole with non-Abelian hair is found for a special value of the Chern-Simons coupling constant.

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